The High Resolution Telescope Cluster. I - Overview and technical status

Details The High Resolution Telescope Cluster. I - Overview and technical status The High Resolution Telescope Cluster. I - Overview and technical status

Jan 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992spie.1546..353w&link_type=abstract

In: Multilayer and grazing incidence X-ray/EUV optics; Proceedings of the Meeting, San Diego, CA, July 22-24, 1991 (A93-39658 15

Physics

Optics

1

Chromosphere, Extreme Ultraviolet Radiation, Far Ultraviolet Radiation, Solar Atmosphere, X Ray Telescopes, High Resolution, Solar Observatories, Spaceborne Telescopes, Spatial Resolution

Scientific paper

A major component of the Advanced Solar Observatory is the High Resolution Telescope Cluster (HRTC) for investigations of the solar atmosphere at soft X-ray, XUV, EUV, and VUV wavelengths, via high resolution spectroheliograms in lines and continuum emitted over the full, (4500 to 100,000,000 K) range of temperatures of the outer solar atmosphere; angular resolution may be as high as 0.03 arcsec. An analysis is conducted of a model HRTC instrument complement encompassing a 60-90 cm aperture VUV telescope, a 40-50 cm aperture EUV telescope, three 40-50 cm aperture XUV telescopes, and a 40-cm aperture soft X-ray telescope, as well as flare spectrometers and polarimeters and four coronagraph/spectrographs.

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